Basic XPS Information Section

The Basic XPS Information Section provides fundamental XPS spectra, BE values, FWHM values, BE tables, overlays of key spectra, histograms and a table of XPS parameters.
The Advanced XPS Information Section is a collection of additional spectra, overlays of spectra, peak-fit advice, data collection guidance, material info,
common contaminants, degradation during analysis, auto-oxidation, gas capture study, valence band spectra, Auger spectra, and more.
Published literature references, and website links are summarized at the end of the advanced section.

→  Periodic Table – HomePage                   XPS Database of Polymers               → Six (6) BE Tables



Potassium (K)

Kalium

Challacolloite – KPb2Cl5 Potassium Metal – Ko Sylvite – KCl

 

  Page Index
  • Peak-fits and Overlays of Rb Chemical Compounds
  • Expert Knowledge & Explanations


Potassium (Ko) Metal

Peak-fits, BEs, FWHMs, and Peak Labels

 


  .
Potassium Metal (Ko)
K (2p) Spectrum – raw
Ion etched clean
Flood Gun OFF – conductive metal
Potassium Metal (Ko)
K (2p) Spectrum – peak-fit
Ion etched clean
Flood Gun OFF – conductive metal
.


Potassium Metal (Ko)
K (2p) extended range
Ion etched clean
Flood Gun OFF – conductive metal
Potassium Metal (Ko)
K (2s) Spectrum – peak-fit
Ion etched clean
Flood Gun OFF – conductive metal

 

 Survey Spectrum of Potassium (Ko) Metal
with Peaks Integrated, Assigned and Labelled

 Periodic Table


 

XPS Signals for Potassium, (Ko) Metal

Spin-Orbit Term,  BE (eV) Value, and Scofield σ for Potassium Kα X-rays (1486 eV, 8.33 Ang)

Overlaps Spin-Orbit Term BE (eV) Value Scofield σ from 1486 eV X-rays IMFP (TPP-2M) in Å
K (2s) 389 2.27 59.1
K (2p1/2) 296.88 1.35 62.6
C (1s) C-F overlaps K (2p3/2) 294.07 2.62 73.7
K (3s) 41 0.286 73.7
O (2s) overlaps K (3p ) 25 0.362 74.4

σ:  abbreviation for the term Scofield Photoionization Cross-Section which are used with IMFP and TF to produce RSFs and atom% quantitation

Plasmon Peaks

Energy Loss Peaks

Auger Peaks

Energy Loss Peak for Compounds:  ~xx eV above each peak max
Intrinsic Bulk Plasmon Peaks:  ~x eV steps
Expected Bandgap for KF: ~  6-6.5 eV   

*Scofield Cross-Section (σ) for C (1s) = 1.0

 Periodic Table 



Plasmon Peaks from Ko Metal

Fresh exposed bulk produced by extensive Ar+ ion etching
  .
K (2p) – Extended Range Spectrum K (2p) – Extended Range Spectrum – Vertically Expanded

 

K (KLL) Auger Peaks from Ko Metal
Fresh exposed bulk produced by extensive Ar+ ion etching

Ko Metal – High resolution Auger peaks Ko Metal – same Auger peaks but taken from Survey spectrum

 

Side-by-Side Comparison of

Potassium (K) and Potassium Halides
Peak-fits, BEs, FWHMs, and Peak Labels


  

 Pure Metal, Ko Potassium Fluoride, KF   
K (2p) from Potassium metal – raw
Ion Etched
Peak-fit of K (2p) from KF
freshly cleaved in lab air
Charge Referenced to 285.0 eV

.
Potassium Fluoride, KF
Peak-fit of K (2p) from KF
freshly cleaved in lab air
Charge Referenced to 285.0 eV
Potassium Chloride, KCl
Peak-fit of K (2p) from KCl, xtal
freshly cleaved in lab air
Charge Referenced to 285.0 eV


.
Potassium Bromide, KBr
Peak-fit of K (2p) from KBr, xtal

freshly cleaved in lab air
Charge Referenced to 285.0 eV
Potassium Iodide, KI
Peak-fit of K (2p) from KI xtal
freshly cleaved in lab air
Charge Referenced to 285.0 eV


Overlay of K (2p) Peak
from Potassium, Ko, KF, and KI

 


 

 

Survey Spectrum of Potassium Fluoride, KF
with Peaks Integrated, Assigned and Labelled

 


 


Survey Spectrum of Potassium Chloride, KCl

with Peaks Integrated, Assigned and Labelled

 


 


Survey Spectrum of Potassium Bromide, KBr
with Peaks Integrated, Assigned and Labelled

 


 


Survey Spectrum of Potassium Iodide, KI
with Peaks Integrated, Assigned and Labelled

 

 


 

Overlay Study of
Carbonate and Bi-Carbonate Chemical Groups

Overlay of C (1s) Spectra from K2CO3 and KHCO3


Potassium Carbonate, K2CO3
Peak-fit of C (1s) from K2CO3, powder
pressed onto stage
Charge Referenced to 285.0 eV

Potassium Hydrogen Carbonate, KHCO3   (potassium bi-carbonate)
Peak-fit of C (1s) from KHCO3, crystallites
freshly crushed
Charge Referenced to 285.0 eV



Overlay of C (1s) Spectra
from K2CO3 and KHCO3



Overlay of K (2p) Spectra
 from K2CO3 and KHCO3

Potassium Carbonate, K2CO3

Peak-fit of K (2p) Spectrum from K2CO3, powder
pressed onto stage
Charge Referenced to 285.0 eV

Potassium Hydrogen Carbonate,
KHCO(potassium bi-carbonate)
Peak-fit of K (2p) Spectrum from KHCO3, crystallites
freshly crushed
Charge Referenced to 285.0 eV
   

Overlay of K (2p) Spectra
 from K2CO3 and KHCO3

 

Valence Band Spectra

K2CO3 and KHCO3

K2CO3 Valence Band Spectrum KHCO3 Valence Band Spectrum
 
 Overlay of Valence Band Spectra
K2CO3 and KHCO3 
Expanded View of Valence Band Spectra

 

Features Observed

  • xx
  • xx
  • xx


Valence Band Spectra

KF, KCl, KBr, KI

KF Valence Band
Spectrum
KCl Valence Band
Spectrum

 


KBr Valence Band
Spectrum
KI Valence Band
Spectrum

Overlay of Valence Band Spectra
KF, KCl, KBr and KI 

 

 

Copyright ©:  The XPS Library



 

Potassium Minerals, Gemstones, and Chemical Compounds

 

Carnallite – KMgCl3 · 6H2O Saltonseaite – K3NaMnCl6 Kainite – KMg(SO4)Cl · 3H2O Chlorothionite – K2Cu(SO4)Cl2

 Periodic Table 

 



 

Six (6) Chemical State Tables of K (2p) BEs

 

  • The XPS Library Spectra-Base
  • PHI Handbook
  • Thermo-Scientific Website
  • XPSfitting Website
  • Techdb Website
  • NIST Website

 



 

Notes of Caution when using Published BEs and BE Tables from Insulators and Conductors:

  • Accuracy of Published BEs
    • The accuracy depends on the calibration BEs used to calibrate the energy scale of the instrument.  Cu (2p3/2) BE can vary from 932.2 to 932.8 eV for old publications
    • Different authors use different BEs for the C (1s) BE of the hydrocarbons found in adventitious carbon that appears on all materials and samples.  From 284.2 to 285.3 eV
    • The accuracy depends on when the authors last checked or adjusted their energy scale to produce the expected calibration BEs
  • Worldwide Differences in Energy Scale Calibrations
    • For various reasons authors still use older energy scale calibrations
    • Some authors still adjust their energy scale so Cu (2p3/2) appears at 932.2 eV or 932.8 eV because this is what the maker taught them
    • This range causes BEs in the higher BE end to be larger than expected
    • This variation increases significantly above 600 eV BE
  • Charge Compensation
    • Samples that behave as true insulators normally require the use of a charge neutralizer (electron flood gun with or without Ar+ ions) so that the measured chemical state spectra can be produced without peak-shape distortions or sloping tails on the low BE side of the peak envelop.
    • Floating all samples (conductive, semi-conductive, and non-conductive) and always using the electron flood gun is considered to produce more reliable BEs and is recommended.
  • Charge Referencing Methods for Insulators
    • Charge referencing is a common method, but it can produce results that are less reliable.
    • When an electron flood gun is used, the BE scale will usually shift to lower BE values by 0.01 to 5.0 eV depending on your voltage setting. Normally, to correct for this flood gun induced shift, the BE of the hydrocarbon C (1s) peak maximum from adventitious carbon is used to correct for the charge induced shift.
    • The hydrocarbon peak is normally the largest peak at the lowest BE.
    • Depending on your preference or training, the C (1s) BE assigned to this hydrocarbon peak varies from 284.8 to 285.0 eV.  Other BEs can be as low as 284.2 eV or as high as 285.3 eV
    • Native oxides that still show the pure metal can suffer differential charging that causes the C (1s) and the O (1s) and the Metal Oxide BE to be larger
    • When using the electron flood gun, the instrument operator should adjust the voltage and the XY position of the electron flood gun to produce peaks from a strong XPS signal (eg O (1s) or C (1s) having the most narrow FWHM and the lowest experimentally measured BE.

 →  Periodic Table 


Table #1

K (2p3/2) Chemical State BEs from:  The XPS Library Spectra-Base”

C (1s) BE = 285.0 eV for TXL BEs
and C (1s) BE = 284.8 eV for NIST BEs

Element Atomic # Compound As-Measured by TXL or NIST Average BE Largest NIST BE Hydrocarbon C (1s) BE  Source
K 19 K-2Ti4O9 292.4 eV 285.0 eV The XPS Library
K 19 K-F (N*3) 292.5 eV 293.1 eV Avg BE – NIST
K 19 K-2O 292.7 eV 292.9 eV 285.0 eV The XPS Library
K 19 K-ClO4 (N*2) 292.8 eV 293.4 eV Avg BE – NIST
K 19 K-Cl 292.9 eV 285.0 eV The XPS Library
K 19 K-Br 293.0 eV 285.0 eV The XPS Library
K 19 K-2SO4 (N*1) 293.3 eV Avg BE – NIST
K 19 K-C8 (N*1) 294.4 eV Avg BE – NIST
K 19 K -element (N*1) 294.7 eV Avg BE – NIST
K 19 K-CN (N*1) 294.7 eV Avg BE – NIST
K 19 K-2CO3 285.0 eV The XPS Library
K 19 K-HCO3 285.0 eV The XPS Library

 (N*number) identifies the number of NIST BEs that were averaged to produce the BE in the middle column.

  • Binding Energy Scale Calibration expects Cu (2p3/2) BE = 932.62 eV and Au (4f7/2) BE = 83.98 eV.  BE (eV) Uncertainty Range:  +/- 0.2 eV
  • Charge Referencing of insulators is defined such that the Adventitious Hydrocarbon C (1s) BE (eV) = 285.0 eV.  NIST uses C (1s) BE = 284.8 eV 
  • Note:   Ion etching removes adventitious carbon, implants Ar (+), changes conductivity of surface, and degrades chemistry of various chemical states.
  • Note:  Ion Etching changes BE of C (1s) hydrocarbon peak.
  • TXL – abbreviation for: “The XPS Library” (https://xpslibrary.com).  NIST:  National Institute for Science and Technology (in USA)

 →  Periodic Table 


Table #2

K (2p3/2) Chemical State BEs from:  “PHI Handbook”

C (1s) BE = 284.8 eV

 

Copyright ©:  Ulvac-PHI


Table #3

K (2p3/2) Chemical State BEs from:  Thermo-Scientific” Website

C (1s) BE = 284.8 eV

Chemical state Binding energy, K 2p3/2 (eV)
KCl 292.9
KBr 293.2

Copyright ©:  Thermo Scientific website


Table #4

K (2p3/2) Chemical State BEs from:  “XPSfitting” Website

Chemical State BE Table derived by Averaging BEs in the NIST XPS database of BEs
C (1s) BE = 284.8 eV

 

Copyright ©:  Mark Beisinger

 


Table #5

K (2p3/2) Chemical State BEs from:  “Techdb.podzone.net” Website

 

XPS Spectra – Chemical Shift | Binding Energy
C (1s) BE = 284.6 eV

XPS(X線光電子分光法)スペクトル 化学状態 化学シフト ケミカルシフト

Element Level Compound B.E.(eV) min max
K 2p3/2 KClO3 292.3 ±0.4 291.9 292.6
K 2p3/2 K4P2O7 292.3 ±0.4 291.9 292.6
K 2p3/2 K2Cr2O7 292.5 ±0.5 292.0 292.9
K 2p3/2 K2CrO4 292.6 ±0.3 292.3 292.9
K 2p3/2 Halides 292.8 ±0.3 292.5 293.1
K 2p3/2 KNO3 292.9 ±0.4 292.5 293.2
K 2p3/2 KClO4 293.4 ±0.3 293.1 293.7
K 2p3/2 K3PO4 293.5 ±0.3 293.2 293.8
K 2p3/2 K 294.5 ±0.4 294.1 294.9
K 2p3/2 KCN 294.7 ±0.4 294.3 295.0


 

Histograms of NIST BEs from K (2p3/2)

Important Note:  NIST Database defines Adventitious Hydrocarbon C (1s) BE = 284.8 eV for all insulators.

 

Histogram indicates a mean BE = 292.68 eV for KCl
based on 4 literature BEs
Histogram indicates  a means K (2p) BE = 292.98 eV for KBr
based on 4 literature BEs

 


Table #6

NIST Database of K (2p3/2) Binding Energies

NIST Standard Reference Database 20, Version 4.1

Data compiled and evaluated
by
Alexander V. Naumkin, Anna Kraut-Vass, Stephen W. Gaarenstroom, and Cedric J. Powell
©2012 copyright by the U.S. Secretary of Commerce on behalf of the United States of America. All rights reserved.

Important Note:  NIST Database defines Adventitious Hydrocarbon C (1s) BE = 284.8 eV for all insulators.

 

Element Spectral Line Formula Energy (eV) Reference
K 2p3/2 KNiIO6 291.90  Click
K 2p3/2 K3[Fe(CN)6] 291.90  Click
K 2p3/2 K3[Mn(CN)6] 291.90  Click
K 2p3/2 K4[Fe(CN)6] 291.90  Click
K 2p3/2 K2Cr2O7 292.10  Click
K 2p3/2 K3[Cr(CN)6] 292.10  Click
K 2p3/2 K4P2O7 292.20  Click
K 2p3/2 K4P2O7 292.20  Click
K 2p3/2 K3[Cr(CN)6] 292.25  Click
K 2p3/2 K/TiO2 292.40  Click
K 2p3/2 K2[(Os(O2)(OH)(H2O))2O2] 292.40  Click
K 2p3/2 KCl 292.40  Click
K 2p3/2 KN3 292.50  Click
K 2p3/2 KRhO2 292.50  Click
K 2p3/2 K3PO4 292.50  Click
K 2p3/2 K2SO4 292.50  Click
K 2p3/2 KF 292.50  Click
K 2p3/2 KClO3 292.60  Click
K 2p3/2 K2CrO4 292.60  Click
K 2p3/2 K2MoO4 292.60  Click
K 2p3/2 K(CH3CH2OCS2) 292.60  Click
K 2p3/2 CH3Br/K/Ag 292.60  Click
K 2p3/2 CH3Br/K/Ag 292.60  Click
K 2p3/2 K/TiO2 292.60  Click
K 2p3/2 K2ZrF6 292.60  Click
K 2p3/2 KZrF5.H2O 292.70  Click
K 2p3/2 K2[Os(O2)(OH)4] 292.70  Click
K 2p3/2 KOsO3N 292.70  Click
K 2p3/2 K3[Co(SCH2CH(NH2)COO)3] 292.70  Click
K 2p3/2 K4[(Os(O2)(NO2)2)2O2].6H2O 292.70  Click
K 2p3/2 K2[MoCl6] 292.70  Click
K 2p3/2 K2[PtCl6] 292.70  Click
K 2p3/2 KCl 292.70  Click
K 2p3/2 K3[Rh(SO3)3].2H2O 292.80  Click
K 2p3/2 KI 292.80  Click
K 2p3/2 KClO4 292.80  Click
K 2p3/2 KMnO4 292.80  Click
K 2p3/2 K2Cr2O7 292.80  Click
K 2p3/2 K2NaPdF6 292.80  Click
K 2p3/2 K2MnO4 292.80  Click
K 2p3/2 K4[Rh2Cl4(CH3COO)4] 292.80  Click
K 2p3/2 K2[IrCl6] 292.80  Click
K 2p3/2 K2[IrCl6] 292.80  Click
K 2p3/2 K2[ReCl6] 292.80  Click
K 2p3/2 K2[SnCl6] 292.80  Click
K 2p3/2 K3[RhCl6] 292.80  Click
K 2p3/2 K3[RhCl6] 292.80  Click
K 2p3/2 KCl 292.80  Click
K 2p3/2 KCl 292.80  Click
K 2p3/2 K3ZrF7 292.80  Click
K 2p3/2 KF 292.80  Click
K 2p3/2 K2[PtCl2(CN)4].3H2O 292.90  Click
K 2p3/2 KBr 292.90  Click
K 2p3/2 KBr 292.90  Click
K 2p3/2 KNO3 292.90  Click
K 2p3/2 K/TiO2 292.90  Click
K 2p3/2 K2[IrCl6] 292.90  Click
K 2p3/2 K2[OsCl6] 292.90  Click
K 2p3/2 K3[Rh(SO3)3].2H2O 293.00  Click
K 2p3/2 K2PdBr4 293.00  Click
K 2p3/2 K3[Rh(NO2)3Cl3] 293.00  Click
K 2p3/2 K3[Rh(NO2)3Cl3] 293.00  Click
K 2p3/2 K3PdF6 293.00  Click
K 2p3/2 AlK(SO4)2.12H2O 293.00  Click
K 2p3/2 K0.7(NaCa)0.3(Mg2.84Fe0.02)Al1.2Si2.8O10(OH1.5F0.50) 293.00  Click
K 2p3/2 K0.7(NaCa)0.3(Mg2.84Fe0.02)Al1.2Si2.8O10(OH1.5F0.50) 293.00  Click
K 2p3/2 K/TiO2 293.00  Click
K 2p3/2 KBr 293.00  Click
K 2p3/2 K2[Os(O2)(C2O4)2] 293.00  Click
K 2p3/2 K2PdCl4 293.00  Click
K 2p3/2 K2[OsCl6] 293.00  Click
K 2p3/2 K2[OsCl6] 293.00  Click
K 2p3/2 K2[PdCl6] 293.00  Click
K 2p3/2 K2[PtCl6] 293.00  Click
K 2p3/2 K3[IrCl6] 293.00  Click
K 2p3/2 KAl2(AlSi3O10)2(OH)2 293.03  Click
K 2p3/2 KBr 293.10  Click
K 2p3/2 K2[Pd(NO2)4] 293.10  Click
K 2p3/2 K3[Rh(NO2)6] 293.10  Click
K 2p3/2 K3[Rh(NO2)6] 293.10  Click
K 2p3/2 K[Ir(NO)Cl5] 293.10  Click
K 2p3/2 K2UF6 293.10  Click
K 2p3/2 KF 293.10  Click
K 2p3/2 KNO2 293.20  Click
K 2p3/2 KClO3 293.20  Click
K 2p3/2 K4Fe(CN)6.3H2O 293.20  Click
K 2p3/2 K4Mo2Cl8 293.20  Click
K 2p3/2 K[(N)OsCl4(H2O)] 293.30  Click
K 2p3/2 K2[Pt(CN)4].3H2O 293.30  Click
K 2p3/2 K3[Rh(NO3)6] 293.30  Click
K 2p3/2 K3[Rh(NO3)6] 293.30  Click
K 2p3/2 K2SO4 293.30  Click
K 2p3/2 K/Rh 293.30  Click
K 2p3/2 K0.9(Mg1.56Fe1.14Ti0.11)Al0.96Si3.0O10(OH1.44F0.56) 293.30  Click
K 2p3/2 K0.9(Mg1.56Fe1.14Ti0.11)Al0.96Si3.0O10(OH1.44F0.56) 293.30  Click
K 2p3/2 K4[Rh2Br4(CH3COO)4] 293.30  Click
K 2p3/2 K2[WCl6] 293.30  Click
K 2p3/2 KClO4 293.40  Click
K 2p3/2 K2WO4/Al2O3 293.40  Click
K 2p3/2 K2[Rh2(CH3COO)4(NO2)2] 293.40  Click
K 2p3/2 K2SO3 293.50  Click
K 2p3/2 (K,Ca)2[Mg4.3Fe0.7][Si7.2Al0.8O22](OH)2 293.50  Click
K 2p3/2 K/Ag 293.60  Click
K 2p3/2 K2.8C60/GaAs 293.66  Click
K 2p3/2 K/Co 293.70  Click
K 2p3/2 K/Ag 293.70  Click
K 2p3/2 K/Pd 293.70  Click
K 2p3/2 K3[Co(CN)6] 293.70  Click
K 2p3/2 K4[V(CN)6] 293.70  Click
K 2p3/2 K2[ReCl6] 293.70  Click
K 2p3/2 KSbF6 293.70  Click
K 2p3/2 K/Ni 293.80  Click
K 2p3/2 K0.8C60/Au 293.80  Click
K 2p3/2 K1.4C60/Au 293.80  Click
K 2p3/2 K2.0C60/Au 293.80  Click
K 2p3/2 K2.7C60/Au 293.80  Click
K 2p3/2 K6.3C60/Au 293.80  Click
K 2p3/2 K6C60/GaAs 293.90  Click
K 2p3/2 K3.9C60/GaAs 293.90  Click
K 2p3/2 Al0.041Si0.264Na0.04K0.02O0.635 294.10  Click
K 2p3/2 K/Ni 294.15  Click
K 2p3/2 K/Ag 294.20  Click
K 2p3/2 K2NiF6 294.20  Click
K 2p3/2 K/Ni 294.35  Click
K 2p3/2 CH3Br/K/Ag 294.40  Click
K 2p3/2 K/Ag 294.50  Click
K 2p3/2 K/Ag 294.50  Click
K 2p3/2 K 294.70  Click
K 2p3/2 KCN 294.70  Click
K 2p3/2 K2.8C60/GaAs 294.83  Click
K 2p3/2 K0.8C60/Au 294.90  Click
K 2p3/2 K1.4C60/Au 294.90  Click
K 2p3/2 K2.0C60/Au 294.90  Click
K 2p3/2 K2.7C60/Au 294.90  Click
K 2p3/2 K6.3C60/Au 294.90  Click

 

 



 

 

Statistical analysis of Binding Energies in NIST Database of BEs

 



 

Advanced XPS Information Section

 

Spectra, BEs, Features, Guidance and Cautions  

for XPS Research Studies on Potassium Materials

 


 

Expert Knowledge Explanations

 

Overlay reveals shift Shake-up Example Auger signal overlaps X


 

XPS Spectra

from

Common Potassium Compounds

                           


 

 

Potassium Oxide, KO2  (Super-oxide)
lump, fresh cut

 

Survey Spectrum  K (2p) Chemical State Spectrum 

 


 

 
C (1s) Chemical State Spectrum  O (1s) Chemical State Spectrum 

 


Valence Band Spectrum from KO2 O Auger Spectrum from KO2

 


 

Potassium Permanganate, KMnO4
crystallite, crushed

Survey Spectrum  K (2p) Chemical State Spectrum 

 


 

 
Mn (2p) Chemical State Spectrum  O (1s) Chemical State Spectrum 

 


 

 
C (1s) Chemical State Spectrum  Valence Band Chemical State Spectrum
  • xx
  • xx
  • xx

 Periodic Table 

Copyright ©:  The XPS Library

 

Potassium Ferricyanide, K3Fe(CN)6
crystal, freshly exposed bulk,  Fe (II)
conductive, Flood Gun ON, NO Charge Correction

Survey Spectrum  K (2p) Chemical State Spectrum

 


 

 
Fe (2p) Chemical State Spectrum
Flood Gun ON, NO Charge Correction
N (1s) Chemical State Spectrum
Flood Gun ON, NO Charge Correction

 


 

 
C (1s) Chemical State Spectrum 
Flood Gun ON, NO Charge Correction
Valence Band Chemical State Spectrum
Flood Gun ON, NO Charge Correction

 


Fe (2p3/2 and 2p1/2) Chemical State Spectrum from K3Fe(CN)6
Simple Fit – Not Optimized

Flood Gun ON, NO Charge Correction

  • xx
  • xx
  • xx

 Periodic Table 



 

Quantitation Details and Information

Quantitation by XPS is often incorrectly done, in many laboratories, by integrating only the main peak, ignoring the Electron Loss peak, and the satellites that appear as much as 30 eV above the main peak.  By ignoring the electron loss peak and the satellites, the accuracy of the atom% quantitation is in error.

When using theoretically calculated Scofield cross-section values, the data must be corrected for the transmission function effect, use the calculated TPP-2M IMFP values, the pass energy effect on the transmission function, and the peak area used for calculation must include the electron loss peak area, shake-up peak area, multiplet-splitting peak area, and satellites that occur within 30 eV of the main peak.

 

Quantitation from Pure, Homogeneous Binary Compound
composed of KF

This section is focused on measuring and reporting the atom % quantitation that results by using:

  • Scofield cross-sections,
  • Spectra corrected to be free from Transmission Function effects
  • A Pass Energy that does not saturate the detector system in the low KE range (BE = 1000-1400 eV)
  • A focused beam of X-ray smaller than the field of view of the lens
  • An angle between the lens and the source that is ~55 deg that negates the effects of beta-asymmetry
  • TPP-2M inelastic mean free path values, and
  • Either a linear background or an iterated Shirley (Sherwood-Proctor) background to define peak areas

The results show here are examples of a method being developed that is expected to improve the “accuracy” or “reliability” of the atom % values produced by XPS.

 

Copyright ©:  The XPS Library  



 

XPS Facts, Guidance & Information

 Periodic Table 

    Element Potassium (K)
 
    Primary XPS peak used for Peak-fitting : K (2p3/2)  
    Spin-Orbit (S-O) splitting for Primary Peak: Spin-Orbit splitting for K (2p) orbital is: 2.9 eV
 
    Binding Energy (BE) of Primary XPS  Signal: 294 eV
 
    Scofield Cross-Section (σ) Value: K (2p3/2) = 2.62     K (2p1/2) = 1.35
 
    Conductivity: Potassium Resistivity = xx
K2CO3 Resistivity = xx
 
    Range of K (2p) Chemical State BEs: 294 – 295 eV range   (Ko to KF)  
signals from other elements that overlap
K (2p) Primary Peak:
  xx
Bulk Plasmons:  
Shake-up Peaks: xx
Multiplet Splitting Peaks:   not possible

 

 

General Information about
Potassium Compounds:
  xx  
Cautions – Chemical Poison Warning

Flammable in water

Copyright ©:  The XPS Library 



 

Information Useful for Peak-fitting K (2p3/2)

  • FWHM (eV) of Pure Potassium metal:  0.8 eV using 25 eV Pass Energy after ion etching and very fast data collection cycles
  • FWHM (eV) of Potassium Halides:  1.3 eV using 50 eV Pass Energy  (before ion etching)
  • Binding Energy (BE) of Primary signal used for Measuring Chemical State Spectra:  294 eV for K (2p) with +/- 0.2 uncertainty
  • List of XPS Peaks that can Overlap Peak-fit results for K (2p):  xx

 Periodic Table 


 

General Guidelines for Peak-fitting XPS signals

  • Typical Energy Resolution for Pass Energy (PE) setting used to measure Chemical State Spectra on Various XPS Instruments
    • Ag (3d5/2) FWHM (eV) = ~0.95 eV for PE 50 on Thermo K-Alpha
    • Ag (3d5/2) FWHM (eV) = ~1.00 eV for PE 80 on Kratos Nova
    • Ag (3d5/2) FWHM (eV) = ~0.95 eV for PE 45 on PHI VersaProbe
    • Ag (3d5/2) FWHM (eV) = ~0.85 eV for PE 50 on SSI S-Probe
  • FWHM (eV) of Pure Elements: Ranges from 0.4 to 1.0 eV across the periodic table
  • FWHM of Chemical State Peaks in any Chemical Compound:  Ranges from 1.1 to 1.6 eV  (in rare cases FWHM can be 1.8 to 2.0 eV)
  • FWHM of Pure Element versus FWHM of Metal Oxide:  Pure element FWHM << Metal Oxide FWHM  (e.g. 0.8 vs 1.5 eV, roughly 2x)
  • If FWHM Greater than 1.6 eV:  When a peak FWHM is larger than 1.6 eV, it is best to add another peak to the peak-fit envelop.
  • BE (eV) Difference in Chemical States: The difference in chemical state BEs is typically 1.0-1.3 eV apart.  In rare cases, <0.8 eV.
  • Number of Peaks to Use:  Use minimum. Do not use peaks with FWHM < 1.0 eV unless it is a metal or a conductive compound.
  • Typical Peak-Shape:  80% G: 20% L,   1.4 eV Gaussian and 0.5 eV Lorentzian
  • Spin-Orbit Splitting of Two Peaks (due to Coupling):  The ratio of the two (2) peak areas must be constrained.
  • Constraints used on Peak-fitting: typically constrain the peak area ratios based on the Scofield cross-section values
  • Asymmetry for Conductive materials:  20-30% with increased Lorentzian %
  • Peak-fitting “2s” or “3s” Peaks:  Often need to use 50-60% Lorentzian peak-shape
  • Notes:
    • Other Oxidation States can appear as small peaks when peak-fitting
    • Pure element signals normally have asymmetric tails that should be included in the peak-fit.
    • Gaseous state materials often display asymmetric tails due to vibrational broadening.
    • Peak-fits of C (1s) in polymers include an asymmetric tail when the energy resolution is very high.
    • Binding energy shifts of some compounds are negative due to unusual electron polarization.

 Periodic Table 


 

Contaminants Specific to Potassium Metal

  • Potassium metal develops a Native oxide that is usually 8-9 nm thick.  .
  • With heat the Native oxide becomes thicker and the BE of the oxide shifts to higher BE
  • Potassium does not readily form a carbide when the surface is ion etched inside the analysis chamber

 

Commonplace Contaminants

  • Carbon and Oxygen are common contaminants that appear on nearly all surfaces. The amount of Carbon usually depends on handling.
  • Carbon is usually the major contaminant.  The amount of carbon ranges from 5-50 atom%.
  • Carbon contamination is attributed to air-borne organic gases that become trapped by the surface, oils transferred to the surface from packaging containers, static electricity, or handling of the product in the production environment.
  • Carbon contamination is normally a mixture of different chemical states of carbon (hydrocarbon, alcohol or ether, and ester or acid).
  • Hydrocarbon is the dominant form of carbon contamination. It is normally 2-4x larger than the other chemical states of carbon.
  • Carbonate peaks, if they appear, normally appear ~4.5 eV above the hydrocarbon C (1s) peak max BE.
  • Low levels of Carbonate is common on many metals that readily oxidize in the air.
  • High levels of Carbonate appear on reactive metal oxides and various hydroxides.  This is due to reaction between the oxide and CO2 in the air.
  • Hydroxide contamination peak is due to the reaction with residual water in the lab air or the vacuum.
  • The O (SO) BE of the hydroxide (water) contamination normally appears 0.5 to 1.0 eV above the oxide peak
  • Potassium (K), Potassium (K), Sulfur (S) and Chlorine (Cl) are common trace to low level contaminants
  • To find low level contaminants it is very useful to vertically expand the 0-600 eV region of the survey spectrum by 5-10X
  • A tiny peak that has 3 or more adjacent data-points above the average noise of the background is considerate to be a real peak
  • Carbides can appear after ion etching various reactive metals.  Carbides form due to the residual CO and CH4 in the vacuum.
  • Ion etching can produce low oxidation states of the material being analyzed.  These are newly formed contaminants.
  • Ion etching polymers by using standard Ar+ ion guns will destroy the polymer, converting it into a graphitic type of carbon

 Periodic Table 


 

Data Collection Guidance

  • Chemical state differentiation can be difficult
  • Long time exposures (high dose) to X-rays can degrade various polymers, catalysts, high oxidation state compounds
  • During XPS analysis, water or solvents can be lost due to high vacuum or irradiation with X-rays or Electron flood gun
  • Auger signals can sometimes be used to discern chemical state shifts when XPS shifts are very small

 Periodic Table 


 

Data Collection Settings for K (2p3/2)

  • Conductivity:  Metal readily develops a native oxide that is sensitive to Flood Gun – Differential Charging Possible – float sample recommended
  • Primary Peak (XPS Signal) used to measure Chemical State Spectra:  K (2p3/2) at 294 eV
  • Recommended Pass Energy for Measuring Chemical State Spectrum: 50-60 eV    (Produces Ag (3d5/2) FWHM ~0.7 eV)
  • Recommended # of Scans for Measuring Chemical State Spectrum:  4-5 scans normally   (Use 10-25 scans to improve S/N)
  • Dwell Time:  50 msec/point
  • Step Size:  0.1 eV/point   (0.1 eV/step or 0.1 eV/channel)
  • Standard BE Range for Measuring Chemical State Spectrum:  288 – 318 eV
  • Recommended Extended BE Range for Measuring Chemical State Spectrum:  275 – 355 eV
  • Recommended BE Range for Survey Spectrum:  -10 to 1,100 eV   (above 1,100 eV there are no useful XPS signals, except for Ge, As and Ga, above 1100 is waste of time)
  • Typical Time for Survey Spectrum:  3-5 minutes for newer instruments, 5-10 minutes for older instruments
  • Typical Time for a single Chemical State Spectrum with high S/N:  5-10 minutes for newer instruments, 10-15 minutes for older instruments  

 Periodic Table 


 

Effects of Argon Ion Etching

  • Carbides can appear after ion etching various reactive metals.  Carbides form due to the residual CO and CH4 in the vacuum.
  • Ion etching can produce low oxidation states of the material being analyzed.  These are newly formed contaminants.
  • Ion etching polymers by using standard Ar+ ion guns will destroy the polymer, converting it into a graphitic type of carbon

 

 Periodic Table 



Gas Phase XPS or UPS Spectra



Chemical State Spectra for K (2p) Published in the Literature
from Thermo Web site
  • Weaker K2p peaks can be easily confused with either C1s (CF2) peaks or C1s satellite structure in aromatic compounds.
    • Assignment of K2p versus C1s feature is possible by identifying spin-orbit components expected for K2p. Also check for K2s peak, binding energy ~378eV.



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